The Gaia mission has revolutionized our view of the Milky Way and its satellite citizens. The
field of Galactic Archaeology has been piecing together the formation and evolution of the …

We review the field of collisionless numerical simulations for the large-scale structure of the
Universe. We start by providing the main set of equations solved by these simulations and …

ABSTRACT We introduce the 'Engineering Dwarfs at Galaxy Formation's Edge'(EDGE)
project to study the cosmological formation and evolution of the smallest galaxies in the …

We investigate the spatial structure and evolution of star formation and the interstellar
medium (ISM) in interacting galaxies. We use an extensive suite of parsec-scale galaxy …

We present a new suite of cosmological zoom-in hydrodynamical (spatial resolution)
simulations of Milky-Way mass galaxies to study how a varying mass ratio for a Gaia …

We study how star formation is regulated in low-mass field dwarf galaxies (), using
cosmological high-resolution () hydrodynamical simulations. Cosmic reionization quenches …

We show how the interplay between active galactic nuclei (AGNs) and merger history
determines whether a galaxy quenches star formation (SF) at high redshift. We first simulate …

In the standard Lambda cold dark matter paradigm, pure dark matter simulations predict
dwarf galaxies should inhabit dark matter haloes with a centrally diverging density 'cusp' …

EDGE: The Origin of Scatter in Ultra-faint Dwarf Stellar Masses and Surface Brightnesses -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …

The concentration parameter is a key characteristic of a dark matter halo that conveniently
connects the halo's present-day structure with its assembly history. Using 'Dark Sky', a suite …